Scattered UV solar radiation within the clouds of Venus

Details Scattered UV solar radiation within the clouds of Venus Scattered UV solar radiation within the clouds of Venus

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.307..345e&link_type=abstract

Nature (ISSN 0028-0836), vol. 307, Jan. 26, 1984, p. 345-347.

Physics

4

Solar Radiation, Ultraviolet Absorption, Venus Clouds, Absorptivity, Aerosols, Albedo, Sulfur Dioxides, Ultraviolet Spectrophotometers, Venera Satellites, Venus, Clouds, Solar Radiation, Wavelengths, Ultraviolet, Scattering, Observations, Spectra, Albedo, Absorption, Thermal Properties, Atmosphere, Venera 14, Aerosols, Altitude

Scientific paper

Results of photometric measurements performed by the Venera-14 descent probe are presented and discussed. True absorption of UV radiation is present everywhere within the cloud structure but most strongly in the upper clouds. Profiles of the volume absorption coefficient and extinction coefficient of the atmosphere indicate that there are two different absorbers which dominate above and below the 57 km level. The most important absorber above this level is probably particulate matter. The data suggest an approximate 1-10 percent mass of sulfur within the upper clouds. The most important absorber below the 57 km level is probably gas.

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